Coronal Heating by MHD Waves
The heating of the solar chromosphere and corona to the observed high temperatures, imply the presence of ongoing heating that balances the strong radiative and thermal conduction losses expected in the solar atmosphere. It has been theorized for decades that the required heating mechanisms of the chromospheric and coronal parts of the active
Van Doorsselaere, Tom et al.
Fecha de publicación:
12
2020